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1.1 Analyzing Motion by Using Diagrams1.3 Predicting Motion from Graphs 1.4 Predicting Motion from Equations 1.5 Problem-Solving Strategies for Kinematics 1.6 Skier Races Downhill 1.8 Se

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Physics

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For users of the two-volume

edition, Volume 1 includes

Chapters 1–16 and Volume 2

17.7 Charges and Fields,

Electric Field Hockey,

Electric Field of

Dreams 563

*18.2 Charges and Fields 587

18.9 Molecular Motors, Optical Tweezers andApplications, StretchingDNA 607

19.2 Conductivity, Ohm‘s Law,Resistance in a Wire 620

19.3 Battery Voltage 624

19.4 Battery-Resistor Circuit,Signal Circuit 630

19.5 Circuit Constructions Kit(DC Only) 633

20.2 Magnets and Compass,Magnets and

Electromagnets 660

20.9 Faraday‘s ElectromagneticLab 681

21.3 Faraday‘s ElectromagneticLab, Faraday‘s Law, Generator 702

*22.3 Circuit Constructions Kit(AC+DC) 744

23.4 Radio Waves &

ElectromagneticFields 766

29.5 Band Structure, Conductivity 989

29.6 Semiconductors,Conductivity 991

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1.1 Analyzing Motion by Using Diagrams

1.3 Predicting Motion from Graphs

1.4 Predicting Motion from Equations

1.5 Problem-Solving Strategies for

Kinematics

1.6 Skier Races Downhill

1.8 Seat Belts Save Lives

1.9 Screeching to a Halt

1.11 Car Starts, then Stops

1.12 Solving Two-Vehicle Problems

1.13 Car Catches Truck

1.14 Avoiding a Rear-End Collision

2.4 Rocket Blasts Off

2.5 Truck Pulls Crate

2.6 Pushing a Crate up a Wall

2.7 Skier Goes down a Slope

2.8 Skier and Rope Tow

2.9 Pole-Vaulter Vaults

2.10 Truck Pulls Two Crates

2.11 Modified Atwood Machine

3.1 Solving Projectile Motion Problems

3.2 Two Balls Falling

3.3 Changing the x-Velocity

3.4 Projectile x- and y-Accelerations

3.5 Initial Velocity Components

3.6 Target Practice I

3.7 Target Practice II

4.1 Magnitude of Centripetal Acceleration

4.2 Circular Motion Problem Solving

4.3 Cart Goes over Circular Path

4.4 Ball Swings on a String

4.5 Car Circles a Track

4.6 Satellites Orbit

5.1 Work Calculations

5.2 Upward-Moving Elevator Stops

5.3 Stopping a Downward-Moving Elevator

5.4 Inverse Bungee Jumper

5.5 Spring-Launched Bowler

5.6 Skier Speed

5.7 Modified Atwood Machine

6.1 Momentum and Energy Change

6.2 Collisions and Elasticity

6.3 Momentum Conservation and

6.8 Skier and Cart

6.9 Pendulum Bashes Box

6.10 Pendulum Person–Projectile Bowling

7.11 Race between a Block and a Disk

7.12 Woman and Flywheel Elevator: Energy Approach

7.13 Rotoride: Energy Approach

7.14 Ball Hits Bat

8.4 State Variables and Ideal Gas Law

8.5 Work Done by a Gas

8.6 Heat, Internal Energy, and First Law of Thermodynamics

8.12 Cyclic Process: Strategies

8.13 Cyclic Process: Problems

8.14 Carnot Cycle

9.3 Vibrational Energy

9.4 Two Ways to Weigh Young Tarzan

9.5 Ape Drops Tarzan

9.6 Releasing a Vibrating Skier I

9.7 Releasing a Vibrating Skier II

9.8 One- and Two-Spring Vibrating Systems

9.9 Vibro-Ride

9.10 Pendulum Frequency

9.11 Risky Pendulum Walk

10.1 Properties of Mechanical Waves

10.2 Speed of Waves on a String

10.4 Standing Waves on Strings

10.5 Tuning a Stringed Instrument: Standing Waves

10.6 String Mass and Standing Waves

10.7 Beats and Beat Frequency

10.8 Doppler Effect: Conceptual Introduction

10.9 Doppler Effect: Problems

11.1 Electric Force: Coulomb’s Law

11.2 Electric Force: Superposition Principle

11.3 Electric Force: Superposition Principle (Quantitative)

11.4 Electric Field: Point Charge

11.5 Electric Field Due to a Dipole

11.6 Electric Field: Problems

11.9 Motion of a Charge in an Electric Field:

Introduction

11.10 Motion in an Electric Field: Problems

11.11 Electric Potential: Qualitative Introduction

12.1 DC Series Circuits (Qualitative)

12.2 DC Parallel Circuits

12.3 DC Circuit Puzzles

12.4 Using Ammeters and Voltmeters

12.5 Using Kirchhoff’s Laws

12.6 Capacitance

12.7 Series and Parallel Capacitors

12.8 R–CCircuit Time Constants

13.1 Magnetic Field of a Wire

13.2 Magnetic Field of a Loop

13.3 Magnetic Field of a Solenoid

13.4 Magnetic Force on a Particle

13.5 Magnetic Force on a Wire

13.6 Magnetic Torque on a Loop

14.3 The Driven Oscillator

15.1 Reflection and Refraction

15.2 Total Internal Reflection

15.3 Refraction Applications

15.4 Plane Mirrors

15.5 Spherical Mirrors: Ray Diagrams

15.6 Spherical Mirror: The Mirror Equation

15.7 Spherical Mirror: Linear Magnification

15.8 Spherical Mirror: Problems

15.9 Thin-Lens Ray Diagrams

15.10 Converging Lens Problems

15.11 Diverging Lens Problems

15.12 Two-Lens Optical Systems

16.1 Two-Source Interference: Introduction

16.2 Two-Source Interference: Qualitative Questions

16.3 Two-Source Interference: Problems

16.4 The Grating: Introduction and Qualitative Questions

16.5 The Grating: Problems

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Hugh D Young is Emeritus Professor of Physics at Carnegie

Mellon University He earned both his undergraduate and

gradu-ate degrees from that university He earned his Ph.D in

funda-mental particle theory under the direction of the late Richard

Cutkosky He joined the faculty of Carnegie Mellon in 1956 and

retired in 2004 He also had two visiting professorships at the

University of California, Berkeley

Dr Young’s career has centered entirely on undergraduate

education He has written several undergraduate-level textbooks,

and in 1973 he became a coauthor with Francis Sears and Mark

Zemansky for their well-known introductory texts In addition to

his authorship of Sears & Zemansky’s College Physics, he is also

coauthor, with Roger Freedman, of Sears & Zemansky’s University

Physics

Dr Young earned a bachelor’s degree in organ performance

from Carnegie Mellon in 1972 and spent several years as

Associ-ate Organist at St Paul’s Cathedral in Pittsburgh He has played

numerous organ recitals in the Pittsburgh area Dr Young and his

wife, Alice, usually travel extensively in the summer, especially

overseas and in the desert canyon country of southern Utah

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College Physics

Hugh D Young

Carnegie Mellon University

9th Edition

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Director of Development: Michael Gillespie

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Cover Photo Credit: Mike Kemp/Rubberball/Corbis

Credits and acknowledgments borrowed from other sources and reproduced, with

permission, in this textbook appear on the appropriate page within the text or on p C-1

Copyright © 2012, 2007, 1991, Pearson Education, Inc., publishing as

Addison-Wesley, 1301 Sansome Street, San Francisco, CA, 94111 All rights reserved

Manufactured in the United States of America This publication is protected by

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Many of the designations used by manufacturers and sellers to distinguish their

products are claimed as trademarks Where those designations appear in this book,

and the publisher was aware of a trademark claim, the designations have been printed

in initial caps or all caps

Mastering Physics®is a registered trademark, in the U.S and/or other countries, of

Pearson Education, Inc or its affiliates

Library of Congress Cataloging-in-Publication Data

Young, Hugh D

Sears & Zemansky’s college physics.—9th ed / Hugh D Young

p cm

Includes bibliographical references and index

ISBN-13: 978-0-321-73317-7 (alk paper)

ISBN-10: 0-321-73317-7 (alk paper)

1 Physics—Textbooks I Sears, Francis Weston, 1898–1975 College physics

II Title III Title: College physics IV Title: Sears and Zemansky’s college physics

QC23.2.Y68 2012

530—dc22

2010046658College Physics—Complete Edition

ISBN 10: 0-321-73317-7; ISBN 13: 978-0-321-73317-7 (Student edition)

ISBN 10: 0-321-73315-0; ISBN 13: 978-0-321-73315-3 (Exam copy)

1 2 3 4 5 6 7 8 9 10—WBC—14 13 12 11 10

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Chapter 0 Mathematics Review 0-1

Mechanics

Chapter 1 Models, Measurements, and Vectors 1

Chapter 2 Motion along a Straight Line 29

Chapter 3 Motion in a Plane 68

Chapter 4 Newton’s Laws of Motion 99

Chapter 5 Applications of Newton’s Laws 128

Chapter 6 Circular Motion and Gravitation 161

Chapter 7 Work and Energy 188

Chapter 9 Rotational Motion 267

Chapter 10 Dynamics of Rotational Motion 294

Periodic Motion, Waves, and Fluids

Chapter 11 Elasticity and Periodic Motion 333

Chapter 12 Mechanical Waves and Sound 365

Chapter 13 Fluid Mechanics 407

Thermodynamics

Chapter 14 Temperature and Heat 441

Chapter 15 Thermal Properties of Matter 477

Chapter 16 The Second Law of

Thermodynamics 516

Electricity and Magnetism

Chapter 17 Electric Charge and Electric Field 545

Chapter 18 Electric Potential and Capacitance 582

Chapter 19 Current, Resistance, and

Direct-Current Circuits 618

Chapter 20 Magnetic Field and

Magnetic Forces 658

Chapter 21 Electromagnetic Induction 698

Chapter 22 Alternating Current 735

Chapter 23 Electromagnetic Waves and Propagation

of Light 761

Light and OpticsChapter 24 Geometric Optics 803

Chapter 25 Optical Instruments 837

Chapter 26 Interference and Diffraction 862

Modern PhysicsChapter 27 Relativity 899

Chapter 28 Photons, Electrons, and Atoms 932

Chapter 29 Atoms, Molecules, and Solids 971

Chapter 30 Nuclear and High-Energy Physics 1003

Appendix A The International System of Units A-1

Appendix B The Greek Alphabet A-3

Appendix C Periodic Table of the Elements A-4

Appendix D Unit Coversion Factors A-5

Appendix E Numerical Constants and Astronomical

Data A-6Answers to Odd-Numbered Problems A-8

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Problem-Solving Strategies coach students in how to approach specific types of problems.

This text’s uniquely extensive set

of Examples enables students to

explore problem-solving challenges

in exceptional detail

Consistent The Set Up / Solve / Reflect format,

used in all Examples, encourages

students to tackle problems thoughtfully

rather than skipping to the math.

Visual Most Examples employ a diagram—

often a pencil sketch that shows

what a student should draw.

NEW! Video Tutor Solution for Every Example

Each Example is explained and solved by an instructor

in a Video Tutor solution provided in the Study Area

of MasteringPhysics®and in the Pearson eText.

NEW! Mathematics Review Tutorials

MasteringPhysics offers an extensive set of assignable mathematics review tutorials, covering all the areas in which students typically have trouble.

L earn basic and advanced skills that help

solve a broad range of physics problems

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NEW! Passage Problems, which use the same reading-passage format as most MCAT questions, develop students’ ability

to apply physics to a real-world situation (often biological or biomedical in nature)

Problems in MasteringPhysics

Select end-of-chapter problems will now offer

additional support such as problem-solving

strategy hints, relevant math review and practice,

and links to the eText These new enhanced

problems bridge the gap between guided tutorials and traditional homework problems.

D evelop problem-solving confidence through a range

of practice options—from guided to unguided

About 20% of the End-of-Chapter Problems

are new or revised These revisions are driven

by detailed student-performance data gathered

nationally through MasteringPhysics.®

Problem difficulty is indicated by a three-dot ranking

system based on data from MasteringPhysics.

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D eepen knowledge of physics by building

connections to the real world.

NEW! PhET Simulations and Tutorials

76 PhET simulations are provided in the Study Area of the MasteringPhysics®website and in the Pearson eText In addition, MasteringPhysics contains 16 new, assignable PhET-based tutorials

NEW! Video Tutor Demonstrations and Tutorials

“Pause and predict” demonstration videos of key physics concepts

engage students by asking them to submit a prediction before seeing

the outcome These videos are available through the Study Area

of MasteringPhysics and in the Pearson eText A set of assignable

tutorials based on these videos challenge students to transfer their

understanding of the demonstration to a related problem situation.

Biomedically Based End-of-Chapter Problems

To serve biosciences students, the text offers

a substantial number of problems based on biological and biomedical situations.

Throughout the text, captioned photos apply physics to real situations, with particular emphasis

on applications of biomedical and general interest

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NEW! Pre-Built Assignments

For every chapter in the book, MasteringPhysics

now provides pre-built assignments that cover

the material with a tested mix of tutorials and end-of-chapter problems of graded difficulty

Professors may use these assignments as-is or

take them as a starting point for modification

Gradebook

• Every assignment is graded automatically.

• Shades of red highlight vulnerable students and challenging assignments

Gradebook Diagnostics

This screen provides your favorite weekly diagnostics

With a single click, charts summarize the most difficult problems, vulnerable students, grade distribution, and even improvement in scores over the course

Class Performance on Assignment

Click on a problem to see which step your students struggled with most, and even their most common wrong answers Compare results at every stage with the national average or with your previous class

M asteringPhysics is the most effective and widely used online science tutorial, homework, and assessment system available.

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Echolocation in bats 3 BIO

Mars mission mistakes 7Train crash illustrates the importance

of precision in measurement 10Vectors in a caribou’s swim across

a river 14

the world” 32Average speed/average velocity

of a race car 37Negative acceleration of a drag racer 39Human centrifuge 42 BIO

Mechanisms in motor neurons 49 BIO

A car’s three accelerators 72Gravisensing in plant roots 73 BIO

Rate of change of velocity in juggling 77Ballistic spores 79 BIO

Human cannonball as projectile 82Uniform circular motion in global positioningsystems 87

first law 102Tablecloth trick: Inertia 103Bubble chamber image:

Studying particles 107Bacterial propulsion 111 BIO

Biathlete using Newton’s third law 113Rocket launch 115

Tug-of-war 116

Telescope mirror 129Liquid-filled accelerometer 134Rock climber using frictional forces 138Wet saw cutting stone 139

Molecular motors 140 BIO

Centripetal force in bobsledding 163Runner using Newton’s third law 170 BIO

Gravity map of the earth 173

Elasticity of tendons and ligaments 201 BIO

Carrying weight on the head 203 BIO

Energy expended in climbing

El Capitan 207 BIO

Cilia and fluid movement in the inner ear 207 BIO

Grasshopper’s catapult mechanism 208 BIO

Measuring a llama’s oxygen consumption 216 BIO

Work at the molecular scale 216 BIO

Conservation of momentum

in a bowling strike 235Momentum of sumo wrestlers 241Light sail 244

Frog’s legs demonstrating impulse 248 BIO

Center of mass in balancing acrobats 253Jet propulsion in jellyfish 255 BIO

angular velocity 269Velocipede direct-drive bicycle 274Storing energy in a flywheel 277Moon orbiting earth 282

Angular acceleration and the inner ear 303 BIO

Rotating DNA and torque 304 BIO

Oxen turning water-well lift 304Nanoengineered gears 306Andaman earthquake’s effects

on length of day 308Spinning dinner plates 313Rifling in a gun barrel 318

Weighing a fish 336Volume stress and strain shape the embryo 337 BIO

Buoyancy in deep-sea hatchetfish 337 BIO

Strength and elasticity

in a spider’s web 340 BIO

Nanobalance 348Foucault pendulum 353

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Wave generation in a surf pool 368

Superposition of mechanical waves

in water ripples 375

Bone flutes: Standing waves 384

Sound-wave vibrations

in the human ear 386 BIO

Prey location by barn owls 390 BIO

Use of sonar in search of shipwrecks 391

Doppler radar in meteorology 395

in a coffee drink 408

Measuring fluid pressure

in the human eyeball 412 BIO

Snowshoeing to reduce pressure 413

Floating in the Dead Sea 418 BIO

Water flow in plants 422 BIO

Turbulent flow in a meandering river 424

Roof blown off by hurricane 425

Bimaterial strips 447

Snowflakes 455

Heat stroke and hot tubs 457 BIO

Using a calorimeter to measure a cow’s heat

production 458 BIO

Heat conduction in predatory fishes 461 BIO

Hawaiian islands: Built by convective flow 465

Infared images 466 BIO

Solar car 467

of stars 478

Martian dust devil 480

Why aircraft cabins are pressurized 481 BIO

Scuba-diving hazards 483 BIO

High-temperature calibration of a platinum

resistance thermometer 485

Hydrogen affects planet size 489

Venus: An arid furnace 490

Nuclear submarines as steamships 495

Geothermal power in Iceland 518

”Bio-diesel” engines 522How a refrigerator works 523Photosynthesis 530 BIO

Energy cycles of the earth and its organisms 535

Zero-power homes 536

strike 546Salt water conducts electricity 549

”Static cling” in DNA 552 BIO

Atom-smashing with Van de Graaff generators553

Platypus sensing electric fields 558 BIO

Cells sensitive to electrical fields 560 BIO

Fish producing and using an electric field tosense its surroundings 565 BIO

Car acting as a Faraday cage in

an electrical storm 572

cell membrane 583 BIO

Patch clamp technique 586 BIO

Lightning bolt 587Bird perching on power line 589 BIO

Sandia Lab’s capacitor bank discharging 596Capacitors in cardiac defibrillators 604 BIO

Magnetic-levitation trains 622 Electric eels 625 BIO

Electrical signaling and tissue regeneration 629 BIO

Recharging ATP molecules 630 BIO

LED bicycle lights 631Wrist strap grounding electronics worker 643 BIO

magnetic field 661 BIO

Magnetic resonance imaging 664 BIO

Microwave ovens 667Direct-current motors 673Coaxial cable 677Magnetohydrodynamic pump 683

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Chapter 21 Induction cooktop 699

Portable energy pack 705Using an electromagnetic tether to deorbitsatellites 710

Recharging pad for electronic devices 712Using magnetic fields to catch red-light runners 716

Step-down transformers 717Detecting tiny magnetic fields in the brain 719 BIO

L –C circuits in tuning knobs 725

Electric pulse treatments for skin cancer 748 BIO

Power surge protection 749

Cerenkov radiation in a nuclear reactor pool 763

Galaxy in different spectral regions 765 BIO

Ultraviolet vision in animals 765Seedling cells guiding light 781 BIO

Physics of a double rainbow 783The human eye’s response to sunlight 784 BIO

Light polarization in cuttlefish 785 BIO

Photoelastic stress analysis 789

Side-view convex mirrors 811Seeing in focus 816 BIO

Green flash at sunset 817Diamond lenses used in optical data storage 821

Compound eyes 841 BIO

Animals’ focusing mechanisms 842 BIO

Eyeglass lenses 843X-ray telescope 850Telescope mirrors 852

Nonreflective coating on museum cases 872Structural color in butterflies 873 BIO

Phase-contrast microscopy 877 BIO

Using diffraction gratings to measure DNA 880 BIO

Reflection diffraction grating in CDs 880Modern telescopes using

interferometry 888

of reference 901Time at the finish line 906Time travel 909

Space and time 914Nuclear power: 920

Fireworks 941Ruby lasers 951Boron neutron capture therapy for brain cancer 956 BIO

Electron microscopy 961 BIO

DNA double helix: Bonding 984 BIO

Diamonds and graphite 990Electron vacancies

in semiconductors 993Transistor radio 996Using quantum physics to look at living tissues 997 BIO

Penetrating power of different types

of radiation 1012Radiocarbon dating 1017 BIO

Residence time of radionuclides

in the body 1019 BIO

Gamma-ray radiosurgery 1020 BIO

Nuclear medicine: Bone scans 1021 BIO

xvi

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“Is physics hard? Is it too hard for me?” Many students are apprehensive about

their physics course However, while the course can be challenging, almost

cer-tainly it is not too hard for you If you devote time to the course and use that time

wisely, you can succeed

Here’s how to succeed in physics.

1 Spend time studying The rule of thumb for college courses is that you

should expect to study about 2 to 3 hours per week for each unit of credit, in addition to the time you spend in class And budget your time: 3 hours every

other day is much more effective than 33 hours right before the exam The good news is that physics is consistent Once you’ve learned how to tackle one topic, you’ll use the same study techniques to tackle the rest of the course So if you find you need to give the course extra time at first, do so and don’t worry—it’ll pay dividends as the course progresses.

2 Don’t miss class Yes, you could borrow a friend’s notes, but listening and

participating in class are far more effective Of course, participating means

paying active attention, and interacting when you have the chance!

3 Make this book work for you This text is packed with decades of teaching

experience—but to make it work for you, you must read and use it actively Think about what the text is saying Use the illustrations Try to solve the

Examples and the Quantitative and Conceptual Analysis problems on your

own, before reading the solutions If you underline, do so thoughtfully and not

mechanically.

A good practice is to skim the chapter before going to class to get a sense for the topic, and then read it carefully and work the examples after class

4 Approach physics problems systematically While it’s important to attend

class and use the book, your real learning will happen mostly as you work problems—if you approach them correctly Physics problems aren’t math

problems You need to approach them in a different way (If you’re “not good

at math,” this may be good news for you!) What you do before and after ing an equation is more important than the math itself The worked examples

solv-in this book help you develop good habits by consistently followsolv-ing three

steps—Set Up, Solve, and Reflect (In fact, this global approach will help you

with problem solving in all disciplines—chemistry, medicine, business, etc.)

5 Use campus resources If you get stuck, get help Your professor probably

has office hours and email; use them Use your TA or campus tutoring center if you have one Partner with a friend to study together But also try to get

unstuck on your own before you go for help That way, you’ll benefit more

from the help you get.

So remember, you can succeed in physics Just devote time to the job,

work lots of problems, and get help when you need it Your book is here to help Have fun!

SET U P

Think about the physics involved in the

situation the problem describes What

information are you given and what do

you need to find out? Which physics

principles do you need to apply?

Almost always you should draw a

sketch and label it with the relevant

known and unknown information

(Many of the worked examples in this

book include hand-drawn sketches to

coach you on what to draw.)

SOLVE

Based on what you did in Set Up,

identify the physics and appropriate

equation or equations and do the

alge-bra Because you started by thinking

about the physics (and drawing a

dia-gram), you’ll know which physics

equations apply to the situation—

you’ll avoid the “plug and pray” trap

of picking any equation that seems to

have the right variables

R EF LECT

Once you have an answer, ask yourself

whether it is plausible If you

calcu-lated your weight on the Moon to be

10,423 kg—you must have made a

mis-take somewhere! Next, check that your

answer has the right units Finally,

think about what you learned from the

problem that will help you later

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and proven innovations in education research, we have revised and enhanced previous material and added new features focusing on more explicit problem- solving steps and techniques, conceptual understanding, and visualization and modeling skills Our main objectives are to teach a solid understanding of the fundamentals, help students develop critical thinking and quantitative reasoning, teach sound problem-solving skills, and spark the students’ interest in physics with interesting and relevant applications.

This text provides a comprehensive introduction to physics at the beginning college level It is intended for students whose mathematics preparation includes high-school algebra and trigonometry but no calculus The complete text may be taught in a two-semester or three-quarter course, and the book is also adaptable to

a wide variety of shorter courses.

New to This Edition

• New Chapter 0 (Mathematics Review) covers math concepts that students

will need to use throughout the course: Exponents; scientific notation and powers of 10; algebra; direct, inverse, and inverse-square relationships; log- arithmic and exponential functions; areas and volumes; and plane geometry and trigonometry This review chapter includes worked examples and end- of-chapter problems.

• New margin applications include over 40 new biosciences-related

applica-tions with photos added to the text, including those focused on cutting-edge technology BIO icons signify the bio-related applications.

• Changes to the end-of-chapter problems include the following:

15–20% of the problems are new.

Many additional biosciences-related problems.

One set of MCAT-style passage problems added at the end of most

chapters, many of them bio-related.

The addition of new biological and biomedical real-world applications and problems gives this edition more coverage in the biosciences than nearly every other book on the market.

• Over 70 PhET simulations are linked to the Pearson eText and are provided

in the study area of the MasteringPhysics website (with icons in the print text) These powerful simulations allow students to interact productively with the physics concepts they are learning PhET clicker questions are also included

on the Instructor Resource DVD.

• Video Tutors bring key content to life throughout the text:

Dozens of Video Tutors feature “pause-and-predict” tions of key physics concepts and incorporate assessment as the student

demonstra-progresses, to actively engage the student in understanding the key ceptual ideas underlying the physics principles.

con-• Every Worked Example in the book is accompanied by a Video Tutor Solution that walks students through the problem-solving process, pro-

viding a virtual teaching assistant on a round-the-clock basis.

All of these Video Tutors play directly through links within the son eText Many also appear in the Study area within MasteringPhysics.

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• Assignable MasteringPhysics tutorials are based on the Video Tutor Demonstrations and PhET simulations.

Video Tutor Demonstrations will be expanded to tutorials in tering by requiring the student to transfer their understanding to a new

Mas-problem situation so that these will be gradable and distinct from the

“pause and predict” demonstrations alone.

Sixteen new PhET tutorials enable students to not only explore the

PhET simulations but also answer questions, helping them make nections between real-life phenomena and the underlying physics that explain such phenomena.

con-Key Features of College Physics

• A systematic approach to problem solving To solve problems with

confi-dence, students must learn to approach problems effectively at a global level, must understand the physics in question, and must acquire the specific skills needed for particular types of problems The Ninth Edition provides research- proven tools for students to tackle each goal.

• The worked examples all follow a consistent and explicit global solving strategy drawn from educational research This three-step approach puts special emphasis on how to set-up the problem before trying to solve it, and the importance of how to reflect on whether the answer is sensible.

problem-• Worked example solutions emphasize the steps and decisions students often

skip In particular, many worked examples include pencil diagrams: drawn diagrams that show exactly what a student should draw in the set-up

hand-step of solving the problem.

• Conceptual Analysis and Quantitative Analysis problems help the students

practice their qualitative and quantitative understanding of the physics The Quantitative Analysis problems focus on skills of quantitative and propor- tional reasoning—skills that are key to success on the MCATs The CAs and QAs use a multiple-choice format to elicit specific common misconceptions.

• Problem-solving strategies teach the students tactics for particular types of

problems—such as problems requiring Newton’s second law, energy vation, etc.—and follow the same 3-step global approach (set-up, solve, and reflect).

conser-• Unique, highly effective figures incorporate the latest ideas from educational research Extraneous detail has been removed and color used only for strict peda- gogical purposes—for instance, in mechanics, color is used to identify the object

of interest, while all other objects are grayscale Illustrations include helpful blue annotated comments to guide students in ‘reading’ graphs and physics fig- ures Throughout, figures, models, and graphs are placed side by side to help students ‘translate’ between multiple representations Pencil sketches are used

consistently in worked examples to emphasize what students should draw.

• Visual chapter summaries show each concept in words, math, and figures to

reinforce how to ‘translate’ between different representations and address ferent student learning styles.

dif-• Rich and diverse end-of-chapter problem sets The renowned Sears &

Zemansky problems, refined over five decades of use, have been revised, expanded and enhanced for today’s courses, based on data from Mastering- Physics.

• Each chapter includes a set of multiple-choice problems that test the skills

developed by the Qualitative Analysis and Quantitative Analysis problems in the chapter text The multiple-choice format elicits specific common miscon- ceptions, enabling students to pinpoint their misunderstandings.

Trang 24

• The General Problems contain many context-rich problems (also known as

real-world problems), which require students to simplify and model more

complex real-world situations Many problems relate to the field of biology

and medicine; these are all labeled BIO.

• Connections of physics to the student’s world In-margin photos with

explanatory captions provide diverse, interesting, and self-contained examples

of physics at work in the world Many of these real-world “applications” are

also related to the fields of biology and medicine and are labeled BIO.

• Writing that is easy to follow and rigorous The writing is friendly yet

focused; it conveys an exact, careful, straightforward understanding of the

physics, with an emphasis on the connections between concepts.

Instructor Supplements

Note: For convenience, all of the following instructor supplements (except for the

Instructor Resource DVD) can be downloaded from the Instructor Area, accessed

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Instructor Solutions, prepared by A Lewis Ford (Texas A&M University)

and Forrest Newman (Sacramento City College) contain complete and detailed

solutions to all end-of-chapter problems All solutions follow consistently the

same Set Up/Solve/Reflect problem-solving framework used in the textbook.

Download only from the MasteringPhysics Instructor Area or from the Instructor

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The cross-platform Instructor Resource DVD (ISBN 978-0-321-76570-3)

provides a comprehensive library of more than 420 applets from ActivPhysics

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are provided in editable Word format Lecture outlines in PowerPoint are also

included along with over 70 PhET simulations as well as Pause and Predict Video

Tutors and Video Tutor Solutions.

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MasteringPhysics enables instructors to:

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problems and tutoring (through additional multi-step tutorial problems that

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• Choose from a wide range of nationally pre-tested problems that provide accurate estimates of time to complete and difficulty.

• After an assignment is completed, quickly identify not only the problems that were the trickiest for students but the individual problem types where students had trouble.

• Compare class results against the system’s worldwide average for each lem assigned, to identify issues to be addressed with just-in-time teaching.

prob-• Check the work of an individual student in detail, including time spent on each problem, what wrong answers they submitted at each step, how much help they asked for, and how many practice problems they worked.

ActivPhysics OnLineTM (accessed through the Study Area within www masteringphysics.com) provides a comprehensive library of more than 420 tried and tested ActivPhysics applets updated for web delivery using the latest online technologies In addition, it provides a suite of highly regarded applet-based tuto- rials developed by education pioneers Alan Van Heuvelen and Paul D’Alessan- dris Margin icons throughout the text direct students to specific exercises that complement the textbook discussion.

The online exercises are designed to encourage students to confront ceptions, reason qualitatively about physical processes, experiment quantita- tively, and learn to think critically The highly acclaimed ActivPhysics OnLine companion workbooks help students work through complex concepts and under- stand them more clearly More than 420 applets from the ActivPhysics OnLine library are also available on the Instructor Resource DVD for this text.

miscon-The Test Bank contains more than 2,000 high-quality problems, with a range

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ques-Five Easy Lessons: Strategies for Successful Physics Teaching (ISBN

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Student Supplements

The Student Solutions Manual, (ISBN 978-0-321-74769-3), written by Lewis

Ford (Texas A&M University) and Forrest Newman (Sacramento City College), contains detailed, step-by-step solutions to more than half of the odd-numbered end-of-chapter problems from the textbook All solutions consistently follow the same Set Up/Solve/Reflect problem-solving framework used in the textbook, reinforcing good problem-solving behavior.

MasteringPhysics® (www.masteringphysics.com) is a homework, tutorial, and assessment system based on years of research into how students work physics problems and precisely where they need help Studies show that students who use MasteringPhysics significantly increase their scores compared to hand- written homework MasteringPhysics achieves this improvement by providing students with instantaneous feedback specific to their wrong answers, simpler sub-problems upon request when they get stuck, and partial credit for their method(s) This individualized, 24/7 Socratic tutoring is recommended by 9 out

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Pearson eText is available through MasteringPhysics, either automatically

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pur-access to the Internet, Pearson eText comprises the full text, including figures

that can be enlarged for better viewing With eText, students are also able to

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Acknowledgments

I want to extend my heartfelt thanks to my colleagues at Carnegie Mellon for

many stimulating discussions about physics pedagogy and for their support and

encouragement during the writing of several successive editions of this book I

am equally indebted to the many generations of Carnegie Mellon students who

have helped me learn what good teaching and good writing are, by showing me

what works and what doesn’t I’m pleased to acknowledge also the contributors

of problems, applications, and other essential elements for this new edition,

including Ken Robinson, Charlie Hibbard, Forrest Newman, Larry Coleman, and

Biman Das Special thanks are due to the Addison-Wesley people, especially

Laura Kenney and Margot Otway, who brought this all together, and to Nancy

Whilton and Kerry Chapman Thanks also to Jared Sterzer at PreMediaGlobal.

Finally, and most importantly, it is always a joy and a privilege to express my

gratitude to my wife Alice and our children Gretchen and Rebecca for their love,

support, and emotional sustenance during the writing of several successive

edi-tions of this book May all men and women be blessed with love such as theirs.

—H.D.Y.

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Susmita Acharya, Cardinal Stritch University

Hamid Aidinejad, Florida Community College,

Jacksonville

Alice Hawthorne Allen, Virginia Tech

Jim Andrews, Youngstown State University

Charles Bacon, Ferris State University

Jennifer Blue, Miami University

Richard Bone, Florida International University

Phillip Broussard, Covenant College

Young Choi, University of Pittsburgh

Orion Ciftja, Prairie View A&M University

Dennis Collins, Grossmont College

Lloyd Davis, Montreat College

Diana Driscoll, Case Western Reserve University

Laurencin Dunbar, St Louis Community College,

Florissant Valley

Alexander Dzyubenko, California State University,

Bakersfield

Robert Ehrlich, George Mason University

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Adam Johnston, Weber State University

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Technology

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Estella Llinas, University of Pittsburgh, Greensburg

Craig Loony, Merrimack College

Rafael Lopez-Mobilia, University of Texas, San Antonio Barbra Maher, Red Rocks Community College

Dan Mazilu, Virginia Tech Randy McKee, Tallahassee Community College Larry McRae, Berry College

William Mendoza, Jacksonville University Anatoli Mirochnitchenko, University of Toledo Charles Myles, Texas Tech University

Austin Napier, Tufts University Erin O’ Connor, Allan Hancock College Christine O’Leary, Wallace State College Jason Overby, College of Charleston James Pazun, Pfeiffer University Unil Perera, Georgia State University David Potter, Austin Community College Michael Pravica, University of Nevada, Las Vegas Sal Rodano, Harford Community College

Rob Salgado, Dillard University Surajit Sen, SUNY Buffalo Bart Sheinberg, Houston Community College Natalia Sidorovskaia, University of Louisiana Chandralekha Singh, University of Pittsburgh Marlina Slamet, Sacred Heart University Daniel Smith, South Carolina State University Gordon Smith, Western Kentucky University Kenneth Smith, Pennsylvania State University Zhiyan Song, Savannah State University Sharon Stephenson, Gettysburg College Chuck Stone, North Carolina A&T State University George Strobel, University of Georgia

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James Vesenka, University of New England Walter Wales, University of Pennsylvania John Wernegreen, Eastern Kentucky University Dan Whitmire, University of Louisiana, Lafayette Sue Willis, Northern Illinois University

Jaehoon Yu, University of Texas, Arlington Nouredine Zettili, Jacksonville State University Bin Zhang, Arkansas State University

Reviewers and Classroom Testers

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0.1 Exponents 0-1

0.2 Scientific Notation and

Powers of 10 0-30.3 Algebra 0-3

0.4 Direct, Inverse, and Inverse-Square

Relationships 0-60.5 Logarithmic and Exponential

Functions 0-100.6 Areas and Volumes 0-10

0.7 Plane Geometry and

1.3 Standards and Units 3

1.4 Unit Consistency and Conversions 7

1.5 Precision and Significant Figures 9

1.6 Estimates and Orders of Magnitude 11

1.7 Vectors and Vector Addition 12

4.1 Force 994.2 Newton’s First Law 1024.3 Mass and Newton’s Second Law 1044.4 Mass and Weight 109

4.5 Newton’s Third Law 1124.6 Free-Body Diagrams 116

5.1 Equilibrium of a Particle 1285.2 Applications of Newton’s Second Law 1335.3 Contact Forces and Friction 1375.4 Elastic Forces 145

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7

11 12 9

Chapter Work and Energy 188

7.1 An Overview of Energy 188

7.2 Work 192

7.3 Work and Kinetic Energy 196

7.4 Work Done by a Varying Force 200

7.5 Potential Energy 203

7.6 Conservation of Energy 208

7.7 Conservative and Nonconservative

Forces 2127.8 Power 216

Chapter Rotational Motion 267

9.1 Angular Velocity and Angular

Acceleration 2679.2 Rotation with Constant Angular

Acceleration 2709.3 Relationship between Linear and

Angular Quantities 2729.4 Kinetic Energy of Rotation and Moment

of Inertia 2779.5 Rotation about a Moving Axis 281

Chapter Dynamics of Rotational

Motion 29410.1 Torque 29410.2 Torque and Angular Acceleration 29710.3 Work and Power in Rotational Motion 303

10.4 Angular Momentum 30510.5 Conservation of Angular Momentum 30710.6 Equilibrium of a Rigid Body 31110.7 Vector Nature of Angular Quantities 317

Chapter Elasticity and Periodic

Motion 33311.1 Stress, Strain, and Elastic Deformations 33311.2 Periodic Motion 34011.3 Energy in Simple Harmonic Motion 343

11.4 Equations of Simple Harmonic Motion 346

11.5 The Simple Pendulum 35111.6 Damped and Forced Oscillations 354

Chapter Mechanical Waves

and Sound 36512.1 Mechanical Waves 36512.2 Periodic Mechanical Waves 36712.3 Wave Speeds 369

12.4 Mathematical Description

of a Wave 37112.5 Reflections and Superposition 373

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13

14

15 16

13.3 Archimedes’ Principle: Buoyancy 416

13.4 Surface Tension and Capillarity 419

13.5 Fluid Flow 422

13.6 Bernoulli’s Equation 424

13.7 Applications of Bernoulli’s

Equation 42713.8 Real Fluids: Viscosity

and Turbulence 430

Chapter Temperature and Heat 441

14.1 Temperature and Thermal

Equilibrium 44114.2 Temperature Scales 443

15.3 Kinetic Theory of an Ideal Gas 48615.4 Heat Capacities 492

15.5 The First Law of Thermodynamics 49315.6 Thermodynamic Processes 50115.7 Properties of an Ideal Gas 503

Chapter The Second Law

of Thermodynamics 51616.1 Directions of Thermodynamic Processes 516

16.2 Heat Engines 51816.3 Internal Combustion Engines 52116.4 Refrigerators 523

16.5 The Second Law

of Thermodynamics 52616.6 The Carnot Engine: The Most EfficientHeat Engine 527

16.7 Entropy 53116.8 The Kelvin Temperature Scale 53516.9 Energy Resources: A Case Study

in Thermodynamics 536

Chapter Electric Charge and

Electric Field 54517.1 Electric Charge 54517.2 Conductors and Insulators 54817.3 Conservation and Quantization

of Charge 551

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17.6 Calculating Electric Fields 560

17.7 Electric Field Lines 563

17.8 Gauss’s Law and Field Calculations 564

18.6 Capacitors in Series and in Parallel 598

18.7 Electric Field Energy 601

19.2 Resistance and Ohm’s Law 620

19.3 Electromotive Force and Circuits 624

19.4 Energy and Power in Electric

Circuits 62919.5 Resistors in Series and in Parallel 632

19.6 Kirchhoff’s Rules 635

19.7 Electrical Measuring Instruments 640

19.8 Resistance-Capacitance Circuits 640

19.9 Physiological Effects of Currents 642

19.10 Power Distribution Systems 643

Chapter Magnetic Field and Magnetic

Forces 65820.1 Magnetism 65820.2 Magnetic Field and Magnetic Force 660

20.3 Motion of Charged Particles in

a Magnetic Field 66720.4 Mass Spectrometers 66920.5 Magnetic Force on a Current-CarryingConductor 670

20.6 Force and Torque on a Current Loop 673

20.7 Magnetic Field of a Long, StraightConductor 677

20.8 Force between Parallel Conductors 67820.9 Current Loops and Solenoids 68020.10 Magnetic Field Calculations 68220.11 Magnetic Materials 685

Chapter Electromagnetic

Induction 69821.1 Induction Experiments 69821.2 Magnetic Flux 700

21.3 Faraday’s Law 70221.4 Lenz’s Law 70621.5 Motional Electromotive Force 70921.6 Eddy Currents 711

21.7 Mutual Inductance 71221.8 Self-Inductance 71421.9 Transformers 71621.10 Magnetic Field Energy 719

21.11 The R–L Circuit 721 21.12 The L–C Circuit 724

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Chapter Alternating Current 735

22.1 Phasors and Alternating Currents 735

22.2 Resistance and Reactance 738

22.3 The Series R–L–C Circuit 744

22.4 Power in Alternating-Current

Circuits 74822.5 Series Resonance 751

22.6 Parallel Resonance 753

Chapter Electromagnetic Waves 761

23.1 Introduction to Electromagnetic

Waves 76123.2 Speed of an Electromagnetic

Wave 76223.3 The Electromagnetic Spectrum 764

23.4 Sinusoidal Waves 765

23.5 Energy in Electromagnetic Waves 768

23.6 Nature of Light 772

23.7 Reflection and Refraction 774

23.8 Total Internal Reflection 780

23.9 Dispersion 782

23.10 Polarization 783

23.11 Huygen’s Principle 789

23.12 Scattering of Light 791

Chapter Geometric Optics 803

24.1 Reflection at a Plane Surface 803

24.2 Reflection at a Spherical Surface 806

24.3 Graphical Methods for Mirrors 813

24.4 Refraction at a Spherical Surface 815

24.5 Thin Lenses 819

24.6 Graphical Methods for Lenses 825

Chapter Optical Instruments 837

25.1 The Camera 83725.2 The Projector 84025.3 The Eye 84125.4 The Magnifier 84525.5 The Microscope 84725.6 Telescopes 84925.7 Lens Aberrations 852

Chapter Interference and

Diffraction 86226.1 Interference and Coherent Sources 862

26.2 Two-Source Interference of Light 86526.3 Interference in Thin Films 86826.4 Diffraction 873

26.5 Diffraction from a Single Slit 87526.6 Multiple Slits and Diffraction Gratings 879

26.7 X-Ray Diffraction 88226.8 Circular Apertures and Resolving Power 885

26.9 Holography 888

Chapter Relativity 899

27.1 Invariance of Physical Laws 90027.2 Relative Nature of Simultaneity 90327.3 Relativity of Time 905

27.4 Relativity of Length 90927.5 The Lorentz Transformation 91327.6 Relativistic Momentum 91627.7 Relativistic Work and Energy 91927.8 Relativity and Newtonian Mechanics 922

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28.1 The Photoelectric Effect 933

28.2 Line Spectra and Energy Levels 938

28.3 The Nuclear Atom and

the Bohr Model 94328.4 The Laser 950

28.5 X-Ray Production and Scattering 951

28.6 The Wave Nature of Particles 954

28.7 Wave–Particle Duality 957

28.8 The Electron Microscope 961

Chapter Atoms, Molecules,

and Solids 971

29.1 Electrons in Atoms 971

29.2 Atomic Structure 979

29.3 Diatomic Molecules 98329.4 Structure and Properties of Solids 98729.5 Energy Bands 989

29.6 Semiconductors 99029.7 Semiconductor Devices 99229.8 Superconductivity 995

Chapter Nuclear and High-Energy

Physics 100330.1 Properties of Nuclei 100330.2 Nuclear Stability 100830.3 Radioactivity 101130.4 Radiation and the Life Sciences 101730.5 Nuclear Reactions 1021

30.6 Nuclear Fission 102330.7 Nuclear Fusion 102730.8 Fundamental Particles 102830.9 High-Energy Physics 103030.10 Cosmology 1036

Answers to Odd-Numbered Problems A-8Credits C-1

Index I-1

Trang 34

Physics

Trang 36

Mathematics Review

0-1

A study of physics at the level of this textbook requires some basic math

skills The relevant math topics are summarized in this chapter We strongly recommend that you review this material, practice end-of- chapter problems, and become comfortable with these as quickly as possible, so that during your physics course, you can focus on the physics concepts

and procedures that are being introduced, without being distracted by unfamiliarity

with the math being used Note that the beauty of physics cannot be enjoyed if you

do not have adequate mastery of basic mathematical skills.

0.1 Exponents

Exponents are used frequently in physics When we write the superscript 4 is

called an exponent and the base number 3 is said to be raised to the fourth

also be raised to a power—for example, There are special names for the

oper-ation when the exponent is 2 or 3 When the exponent is 2, we say that the

quan-tity is squared; thus, means x is squared When the exponent is 3, the quantity

is cubed; hence, means x is cubed.

Note that and the exponent 1 is typically not written Any quantity raised to the zero power is defined to be unity (that is, 1) Negative exponents are

used for reciprocals: An exponent can also be a fraction, as in

The exponent is called a square root, and the exponent is called a cube root.

For example, can also be written as Most calculators have special keys for calculating numbers raised to a power—for example, a key labeled or

The arrangement of seeds in

a sunflower is a classic ple of how natural processes give rise to patterns that can

exam-be expressed by means of fairly simple mathematics.

In this chapter, we will review most of the mathematics you will need for this course.

Trang 37

Exponents obey several simple rules, which follow directly from the meaning

of raising a quantity to a power:

1 The product rule:

and

2 The quotient rule:

A special case of this rule is,

3 The first power rule:

4 Other power rules:

21 11

Simplify the expression x and calculate its numerical value when x5 6and y5 3

R E F L E C T Notice that we raised both sides of the equation to the

power As explained in Section 0.3, an operation performed onboth sides of an equation does not affect the equation’s validity

1

Trang 38

0.2 Scientific Notation and Powers of 10

In physics, we frequently encounter very large and very small numbers, and it is

important to use the proper number of significant figures when expressing a

phys-ical quantity Both these issues are addressed by using scientific notation, in

which a quantity is expressed as a decimal number with one digit to the left of the

decimal point, multiplied by the appropriate power of 10 If the power of 10 is

positive, it is the number of places the decimal point is moved to the right to

power of 10 is negative, it is the number of places the decimal point is moved

to the left to obtain the fully written-out number For example,

In going from 6.56 to 0.00656, the decimal point is moved three places

to the left, so is the correct power of 10 to use when the number is written in

scientific notation Most calculators have keys for expressing a number in either

decimal (floating-point) or scientific notation.

When two numbers written in scientific notation are multiplied (or divided),

multiply (or divide) the decimal parts to get the decimal part of the result, and

multiply (or divide) the powers of 10 to get the power-of-10 portion of the result.

You may have to adjust the location of the decimal point in the answer to express

it in scientific notation For example,

Similarly,

Your calculator can handle these operations for you automatically, but it is

impor-tant for you to develop good “number sense” for scientific notation manipulations.

When adding, subtracting, multiplying, or dividing numbers, keeping the

proper number of significant figures is important See Section 1.5 to review how

to keep the proper number of significant figures in these cases.

0.3 Algebra

Solving Equations

Equations written in terms of symbols that represent quantities are frequently used

in physics An equation consists of an equal sign and quantities to its left and to

its right Every equation tells us that the combination of quantities on the left of

the equals sign has the same value as (that is, equals) the combination on the right

of the equals sign For example, the equation tells us that

that

Often, one of the symbols in an equation is considered to be the unknown,

and we wish to solve for the unknown in terms of the other quantities For

exam-ple, we might wish to solve the equation for the value of x Or we

might wish to solve the equation for the unknown a in terms of x,

t, and Use the following rule to solve an equation:

An equation remains true if any valid operation performed on one side

of the equation is also performed on the other side The operations could be

(a) adding or subtracting a number or symbol, (b) multiplying or dividing by a

number or symbol, or (c) raising each side of the equation to the same power.

Trang 39

The Quadratic Formula

Using the methods of the previous subsection, we can easily solve the equation

for x:

The equation is also easily solved by factoring out an x on the

left side of the equation, giving (To factor out a quantity means

to isolate it so that the rest of the expression is either multiplied or divided by that quantity.) The equation is true (that is, the left side equals zero)

if either or These are the two solutions of the equation For

and

nonzero, we cannot use the previous simple methods to solve for x Such an

equation is called a quadratic equation, and its solutions are expressed by the quadratic formula:

Solve the equation 2x21 4 5 22for x.

S O L U T I O N

S E T U P A N D S O LV E First we subtract 4 from both sides This

gives Then we divide both sides by 2 to get

Finally, we raise both sides of the equation to the power

(In other words, we take the square root of both sides of the

equa-tion.) This gives x That is, x 3 or x 3

We can verify our answers by substituting our result back into

the original equation:

so x5 63does satisfy the equation

181 4 5 22,

45 2192 1 4 5

2x21 4 5 2163221

25156!9 5 63

5

12

x25 9

2x25 18

R E F L E C T Notice that a square root always has two possible

val-ues, one positive and one negative For instance,because and 2 2 4 Your calculator willgive you only a positive root; it’s up to you to remember thatthere are actually two Both roots are correct mathematically, but

in a physics problem only one may represent the answer Forinstance, if you can get dressed in minutes, the only physi-cally meaningful root is 2 minutes!

!4

522121

Solve the equation x 5 v0t11 for a.

at2

S O L U T I O N

S E T U P A N D S O LV E We subtract from both sides This gives

Now we multiply both sides by 2 and divide both sides by giving

Trang 40

Quadratic formula

For a quadratic equation in the form where a, b, and c are

real numbers and the solutions are given by the quadratic formula:

x 5 2b 6 "b22 4ac

2a

a 2 0,

ax21 bx 1 c 5 0,

Find the values of x that satisfy the equation 2x22 2x 5 24.

so or If x represents a physical quantity that takes

only nonnegative values, then the negative root is physical and is discarded

non-R E F L E C T As we’ve mentioned, when an equation has more than

one mathematical solution or root, it’s up to you to decide whether

one or the other or both represent the true physical answer (If ther solution seems physically plausible, you should review yourwork.)

x5 23

x5 4

Simultaneous Equations

If a problem has two unknowns—for example, x and y—then it takes two

inde-pendent equations in x and y (that is, two equations for x and y, where one

equation is not simply a multiple of the other) to determine their values

uniquely Such equations are called simultaneous equations because you

solve them together A typical procedure is to solve one equation for x in terms

of y and then substitute the result into the second equation to obtain an

equa-tion in which y is the only unknown You then solve this equaequa-tion for y and use

the value of y in either of the original equations in order to solve for x A pair

of equations in which all quantities are symbols can be combined to eliminate

one of the common unknowns In general, to solve for n unknowns, we must

have n independent equations Simultaneous equations can also be solved

graphically by plotting both equations using the same scale on the same graph

paper The solutions are the coordinates of the points of intersection of the

unequal complex numbers and cannot represent physical quantities In such

a case, the quadratic equation has mathematical solutions, but no physical

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